Tuesday, 14 April 2015 15:44 UTC
The speed of the solar wind as well as the interplanetary magnetic field strength and solar wind plasma temperature started to increase early this morning which is likely associated with the expected arrival of a solar wind stream associated with a coronal hole on the Sun's southern hemisphere.
However, the solar wind speed is still slow right now with a speed of about 350 km/s meaning geomagnetic storming conditions should not be expected just yet. The strength of the interplanetary magnetic field is right now about 11nT and it's direction (Bz) is southward at -10nT meaning we will likely see enhanced auroral activity in the hours ahead up to a Kp-value of 4. This stands for active geomagnetic conditions with possible auroral displays visible on the horizon from northern Scotland, Norway, large parts of Sweden and Finland.
A large asymmetric full halo coronal mass ejection became visible early this morning in SOHO/LASCO imagery but it has been determined that it came from a far side event. No effects are expected from this event at Earth.
Image: A far side full halo CME can be seen on this image from SOHO.
Thank you for reading this article! Did you have any trouble with the technical terms used in this article? Our help section is the place to be where you can find in-depth articles, a FAQ and a list with common abbreviations. Still puzzled? Just post on our forum where we will help you the best we can!
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
Whitehorse, YT, Yellowknife, NTA lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
The anticipated strong G3 geomagnetic storm watch never materialized as the coronal mass ejection that was supposed to arrive early yesterday didn't arrive until today just past midnight UTC. The impact was very lackluster with the Bt (total strength of the IMF) increasing to a moderate 15nT at best and the solar wind speed reaching just 420km/s. A far cry from the anticipated 700 to 800km/s. That once again goes to show how hard it is to forecast space weather events and any resulting geomagnetic conditions. We remain under the influence of the CME and high latitude sky watchers should remain alert for some nice aurora displays but middle latitude sky watchers will probably have to wait for the next opportunity.
Read moreA transequatorial coronal hole is facing Earth. Enhanced solar wind could arrive in ~3 days
Active geomagnetic conditions (Kp4) Threshold Reached: 02:33 UTC
Last X-flare | 2025/02/23 | X2.0 |
Last M-flare | 2025/03/21 | M1.2 |
Last geomagnetic storm | 2025/03/22 | Kp6- (G2) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
February 2025 | 154.6 +17.6 |
March 2025 | 138.3 -16.4 |
Last 30 days | 136.1 -18.1 |